Abstract
The present state of knowledge about winds and chromospheres of G, K, and M giants and supergiants has been reviewed.
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References
Dupree, A.K., Reimers, D. 1987, Mass-loss from Cool Stars in Scientific Accomplishments of the IUE (ed. K. Kondo) D. Reidel p. 321–353.
Reimers, D. 1987a, What Do Binaries Teach us about Mass-Loss in Cool Stars in IAU Symp. 122 “Circumste1lar Matter” (I. Appenzeller, C. Jordan eds.), D. Reidel p.307–319.
Reimers, D. 1987b, Winds in Late Type Stars and the Solar Wind, in Solar and Stellar Physics (E.H. Schröter, M. Schüssler eds.) Lecture Notes in Physics, Springer Berlin
Schröder, K.-P. 1985, Astron.Astrophys. 147, l03
Schröder, K.-P. 1986, Astron.Astrophys. 170, 70
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© 1988 Kluwer Academic Publishers
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Reimers, D. (1988). Winds in Cool Stars. In: Havnes, O., Pettersen, B.R., Schmitt, J.H.M.M., Solheim, J.E. (eds) Activity in Cool Star Envelopes. Astrophysics and Space Science Library, vol 143. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-2951-7_48
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DOI: https://doi.org/10.1007/978-94-009-2951-7_48
Publisher Name: Springer, Dordrecht
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